Search for neutrino emission from GRB 221009A using the KM3NeT ARCA and ORCA detectors
- NázevTitle
- Search for neutrino emission from GRB 221009A using the KM3NeT ARCA and ORCA detectorsSearch for neutrino emission from GRB 221009A using the KM3NeT ARCA and ORCA detectors
- Druh výsledkuResult type
- Článek v časopiseJournal article
- AutořiAuthors
- S. Aiello, A. Albert, M. Alshamsi, S. Alves Garre, Z. Bardačová, E. Eckerová, F. Mamedov, Y. Shitov, I. Štekl
- DOIDOI
- 10.1088/1475-7516/2024/08/006
- Časopis / citaceJournal / citation
- JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS. 2024, 2024(8), 1-12. ISSN 1475-7516.
- RokYear
- 2024
- JazykLanguage
- eng
- WoSWoS
- 001371218700001
- ScopusScopus
- 2-s2.0-85200842791
- RIVRIV
- RIV/68407700:21670/24:00377443!RIV25-GA0-21670___
- ProjektProject
- Hodnocení radioaktivity materiálu a vylepšené kalibrační techniky pro zvýšení výkonnosti neutrinových teleskopů KM3NETMaterial radioactivity evaluations and improved calibration techniques to advance performances of the KM3NET neutrino telescopes
AbstraktAbstract
Gamma-ray bursts are promising candidate sources of high-energy astrophysical neutrinos. The recent GRB 221009A event, identified as the brightest gamma-ray burst ever detected, provides a unique opportunity to investigate hadronic emissions involving neutrinos. The KM3NeT undersea neutrino detectors participated in the worldwide follow-up effort triggered by the event, searching for neutrino events. In this paper, we summarize subsequent searches, in a wide energy range from MeV up to a few PeVs. No neutrino events are found in any of the searches performed. Upper limits on the neutrino emission associated with GRB 221009A are computed.
Gamma-ray bursts are promising candidate sources of high-energy astrophysical neutrinos. The recent GRB 221009A event, identified as the brightest gamma-ray burst ever detected, provides a unique opportunity to investigate hadronic emissions involving neutrinos. The KM3NeT undersea neutrino detectors participated in the worldwide follow-up effort triggered by the event, searching for neutrino events. In this paper, we summarize subsequent searches, in a wide energy range from MeV up to a few PeVs. No neutrino events are found in any of the searches performed. Upper limits on the neutrino emission associated with GRB 221009A are computed.